On the Nature of Prominence Bubbles and Plumes

0386695 - ASÚ 2013 RIV US eng C - Conference Paper (international conference)
Schmieder, B. - Zapiór, M. - Heinzel, Petr - Aulanier, G.
On the Nature of Prominence Bubbles and Plumes.
The Fifth Hinode Science Meeting: Exploring the active Sun. San Francisco: Astronomical Society otf the Pacific, 2012 - (Golub, L.), s. 77-78. ASP Conference Series, 456. ISBN 9781583817940.
[Hinode Science Meeting /5./. Cambridge (US), 10.10.2011-14.10. 2011]
Institutional support: RVO:67985815
Keywords : MHD modeling * bubbles * plumes
Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics

An example of bubble and related plume, using time series in selected SDO/AIA channels and co-temporal MSDP observations in the Ha line obtained at Wroclaw-Bialkow observatory on April 20, 2011 is presented. The formation of bubbles may be due to emerging arcades in the filament channel, below the prominence. After discussing on MHD modeling, we conclude that bubbles and plumes are parts of the corona observed through gaps/windows in the prominence.
Permanent Link: http://hdl.handle.net/11104/0216002